D/antiD Dark Energy in String Warped Compactification
Yun-Song Piao

TL;DR
This paper investigates the evolution and decay of relic D3-branes in string warped compactification, highlighting their role in transitioning from de Sitter to anti-de Sitter vacua and their implications for the stability of the universe.
Contribution
It introduces a detailed analysis of D3-brane dynamics post-inflation, revealing a decay mechanism for dS vacua in string theory models.
Findings
D3-branes can be temporarily frozen during radiation/matter domination.
Late-time potential energy causes D3-branes to move towards d-branes.
Annihilation of D3/d-branes results in the disappearance of dS vacua.
Abstract
We study the evolution of relic D3-branes after the D3/\bd-brane inflation in string warped compactification. The motion of D3-branes can be frozen under certain condition during the radiation/matter domination. These D3-branes can not be released until the D3/\bd-branes potential energy becomes dominated at late time. Subsequently they will move towards to \bd-branes, which play the role of uplifting AdS minimum to dS minimum, near the apex of throats. The annihilation of D3/\bd-branes leads to the disappearance of dS vacua. This process may be regarded as a rapid decay channel of present dS vacua. We discuss the parameter spaces required by this process and calculate the decay time.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
